GEOCHEMICAL AND ISOTOPIC COMPOSITION OF APPALACHIAN BASIN BRINES: ORIGIN OF SALINITY AND FINGERPRINTS OF FLUID RESERVOIRS
Produced waters from Marcellus Shale gas wells, after injection of low-TDS hydraulic fracturing fluids and subsequent flowback, are highly saline (14 to 248 g/L TDS). These brines are dominated by Na-Ca-Cl and contain elevated Br concentrations and Br/Cl ratios, indicative of paleoseawater evaporated past halite saturation and further modified by subsequent diagenetic reactions. Variable solute concentrations with relatively constant solute to bromide ratios suggest later brine dilution by freshwater. Oxygen and hydrogen isotopes plot to the right of the Global Meteoric Water Line, along a mixing trend between evapoconcentrated seawater and a meteoric water endmember. Marcellus Shale formation waters have similar major ion chemistry and water stable isotope compositions to adjacent Upper Devonian shales and sandstone formation waters, yet are distinct from brines in underlying Silurian formations and dilute groundwater in shallow aquifers. Strontium isotope ratios of Marcellus Shale brines are less radiogenic than formation waters in overlying shale and sandstone formations. In addition, produced waters from the Marcellus Shale are highly radioactive, with median total radium concentrations greater than non-Marcellus formations and fluids in other sedimentary basins worldwide.